Source Population and Acceleration Location of Suprathermal Heavy Ions in Corotating Interaction Regions
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/838/i=1/a=23/pdf
Reference30 articles.
1. Formation, shape, and evolution of magnetic structures in CIRs at 1 AU
2. Abundances of Suprathermal Heavy Ions in CIRs During the Minimum of Solar Cycle 23
3. Modeling interstellar pickup ion distributions in corotating interaction regions inside 1 AU
4. The suprathermal seed population for corotating interaction region ions at 1 AU deduced from composition and spectra of H+, He++, and He+observed on Wind
5. COMPOSITION AND SPECTRAL PROPERTIES OF THE 1 AU QUIET-TIME SUPRATHERMAL ION POPULATION DURING SOLAR CYCLE 23
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1. Quiet-time Spectra of Suprathermal Heavy Ions near 1 au in Solar Cycles 23 and 24;The Astrophysical Journal Letters;2024-03-28
2. Multispacecraft Energetic Particle Enhancements Associated with a Single Corotating Interaction Region;The Astrophysical Journal;2024-02-01
3. First results from the Solar Orbiter Heavy Ion Sensor;Astronomy & Astrophysics;2023-08
4. Solar Cycle Variation of 0.3–1.29 MeV Nucleon−1 Heavy Ion Composition During Quiet Times Near 1 au in Solar Cycles 23 and 24;The Astrophysical Journal;2023-07-01
5. A Mosaic of the Inner Heliosphere: Three Carrington Rotations During the Whole Heliosphere and Planetary Interactions Interval;Journal of Geophysical Research: Space Physics;2023-06
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